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Title: The Stellar IMF from turbulent fragmentation
Authors: Padoan, P.
Nordlund, A.
Issue Date: 2001
Abstract: In this paper they conclude that turbulent fragmentation is unavoidable in super-sonically turbulent molecular clouds, and given the success of the present model to predict the observed shape of the Stellar IMF, they conclude that turbulent fragmentation is essential to the origin of the stellar IMF.
Appears in Collections:JPL TRS 1992+

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